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Gas signatures of Herbig Ae/Be disks probed with Herschel SPIRE spectroscopy
Published online by Cambridge University Press: 06 January 2014
Abstract
Herbig Ae/Be objects, like their lower mass counterparts T Tauri stars, are seen to form a stable circumstellar disk which is initially gas-rich and could ultimately form a planetary system. We present Herschel SPIRE 460–1540 GHz spectra of five targets out of a sample of 13 young disk sources, showing line detections mainly due to warm CO gas.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 175 - 176
- Copyright
- Copyright © International Astronomical Union 2013